Bayesian Analysis of Hot-Jupiter Radius Anomalies: Evidence for Ohmic Dissipation?

The cause of hot-Jupiter radius inflation, where giant planets with > 1000 K are significantly larger than expected, is an open question and the subject of many proposed explanations. Many of these hypotheses postulate an additional anomalous power that heats planets' convective interiors, l...

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Veröffentlicht in:	The Astronomical journal 2018-05, Vol.155 (5), p.214
Hauptverfasser:	Thorngren, Daniel P., Fortney, Jonathan J.
Format:	Artikel
Sprache:	eng
Schlagworte:	Anomalies Astronomy Bayesian analysis Jupiter Ohmic dissipation Planetary evolution Planets planets and satellites: gaseous planets planets and satellites: interiors planets and satellites: physical evolution Statistical models Thermal evolution
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